Direct Galileo imaging data were obtained of the Jupiter impact sites
for Comet Shoemaker-Levy 9 fragments K, N, and W during their early, h
igh-energy phases. Initial similar to 5s-long flashes for all 3 impact
s result from radiant bolides; analogous, abrupt onsets of luminosity
observed by the Galileo photopolarimeter for other impacts must also b
e the bolide phase. The 3 bolides were dim at 0.56 or 0.89 mu m (few p
ercent of total Jupiter) and had similar amplitudes, despite huge late
-stage differences observed from Earth. Subsequent, continuous luminos
ity lasting similar to 40s for K and similar to 10s for N is optical r
adiation as the initial bolide train erupts into a ''fireball''. The K
light curve may show (a) two impacts 10s apart or (b) delayed evoluti
on of the fireball.